Using the linear approximation for small oscillations, we solve for θ(t) with initial conditions θ(0) = 0.4 radians and dθ/dt (0) = 0.2 rad/s. We determine the angular frequency to find the equation of motion, and use that to calculate the period.
To find the equation of motion for the pendulum, we will be using the linear differential equation d²θ/dt² + (g/L)θ = 0, where g is the acceleration due to gravity (9.8 m/s²) and L is the length of the pendulum (1.5 meters).
First, we recognize this equation resembles the harmonic oscillator equation whose solution has the form θ(t) = Acos(ωt - δ), where ω is the angular frequency and A and δ are determined from initial conditions. Using the initial conditions θ(0) = 0.4 radians and dθ/dt (0) = 0.2 radians per second, we find A and δ. The angular frequency ω can be found from ω² = g/L, leading to ω = √(g/L). Substituting g = 9.8 m/s² and L = 1.5 meters, the angular frequency is ω = √(9.8/1.5).
The period T of the pendulum is found using the formula T = 2π/ω. Plugging in the calculated ω gives us the period for one complete oscillation.